J/ApJ/870/1 PUSH CCSN to explosions in spherical symmetry. II. (Ebinger+, 2019)
PUSHing core-collapse supernovae to explosions in spherical symmetry.
II. Explodability and remnant properties.
Ebinger K., Curtis S., Frohlich C., Hempel M., Perego A., Liebendorfer M.,
Thielemann F.-K.
<Astrophys. J., 870, 1-1 (2019)>
=2019ApJ...870....1E 2019ApJ...870....1E (SIMBAD/NED BibCode)
ADC_Keywords: Supernovae; Stars, masses; Models
Keywords: hydrodynamics; nuclear reactions, nucleosynthesis, abundances
stars: neutron; supernovae: general
supernovae: individual:SN 1987A
Abstract:
In a previously presented proof-of-principle study, we established a
parameterized spherically symmetric explosion method (PUSH) that can
reproduce many features of core-collapse supernovae (CCSN). The
present paper goes beyond a specific application that is able to
reproduce observational properties of SN1987A and performs a
systematic study of an extensive set of nonrotating, solar metallicity
stellar progenitor models in the mass range from 10.8 to 120M☉.
This includes the transition from neutron stars to black holes as the
final result of the collapse of massive stars, and the relation of the
latter to supernovae, possibly faint supernovae, and failed
supernovae. We discuss the explosion properties of all models and
predict remnant mass distributions within this approach. The present
paper provides the basis for extended nucleosynthesis predictions in a
forthcoming paper to be employed in galactic evolution models.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table5.dat 41 111 WHW02 and WH07 models (standard calibration)
--------------------------------------------------------------------------------
See also:
J/ApJ/608/405 : Explosive yields of massive star (Chieffi+, 2004)
J/AJ/131/2245 : BATC photometry of SN2004dj (Zhang+, 2006)
J/MNRAS/372/1315 : UBVRI photometry of SN 2004et (Sahu+, 2006)
J/ApJ/724/341 : Nucleosynthesis of massive metal-free stars (Heger+, 2010)
J/MNRAS/408/827 : Simulations of supernova explosions (Dessart+, 2010)
J/ApJS/199/38 : Presupernova evolution (Limongi+, 2012)
J/ApJ/764/21 : Stellar evolutionary models with 13-120Msun (Chieffi+, 2013)
J/ApJ/769/99 : Nucleosynthetic yields for stars >12M☉ (Brown+, 2013)
J/MNRAS/433/1871 : UBVRI griz light curves of SN 2012aw (Bose+, 2013)
J/ApJ/808/42 : CHemical Abundances of Spirals II. M51 (Croxall+, 2015)
J/ApJ/824/6 : Obs. of precursor to SNHunt275 2015 May event (Ofek+, 2016)
J/A+A/624/A66 : Massive runaway and walkaway stars models (Renzo+, 2019)
Byte-by-byte Description of file: table5.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 5 A5 --- Model Model identifier; WHW02 or WH07 (1)
7- 11 F5.1 Msun Mzams [10/120] Zero-age main sequence (ZAMS) mass
13- 17 F5.2 Msun Mprog [6/17] Progenitor mass
19- 22 F4.2 10+44J Eexpl [0.5/1.7] Explosion energy; in 1051erg units
24- 27 F4.2 s texpl [0.26/0.56] Time of explosion
29- 36 E8.2 Msun MNi [0.02/0.16] Ejected mass of 56Ni
38- 41 F4.2 Msun Mrem [1.3/2] Remnant mass
--------------------------------------------------------------------------------
Note (1): We use two sets of nonrotating pre-explosion models with
solar metallicity from the stellar evolution code KEPLER presented in
WHW02 (Ref 1; Woosley+ 2002RvMP...74.1015W 2002RvMP...74.1015W) and
WH07 (Ref 2; Woosley & Heger 2007PhR...442..269W 2007PhR...442..269W).
Pre-explosion models used in this study (Table 1):
---------------------------------------------------------
Series Label Min Mass Max Mass Deltam Ref
Msun Msun Msun
---------------------------------------------------------
WHW02 s 10.8 28.2 0.2 1
29.0 40.0 1.0 1
75.0 1
WH07 w 12.0 33.0 1.0 2
35.0 60.0 5.0 2
70.0 2
80.0 120.0 20.0 2
---------------------------------------------------------
All models have solar metallicity. Note that the pre-explosion models
are irregularly spaced in mass. The Deltam indicates the mass spacings
of available pre-explosion models for each mass interval Min Mass to
Max Mass.
--------------------------------------------------------------------------------
History: From electronic version of the journal
References:
Perego et al. Paper I. 2015ApJ...806..275P 2015ApJ...806..275P
Curtis et al. Paper III. 2019ApJ...870....2C 2019ApJ...870....2C Cat. J/ApJ/870/2
Ebinger et al. Paper IV. 2020ApJ...888...91E 2020ApJ...888...91E
(End) Prepared by [AAS], Coralie Fix [CDS] 31-Jan-2020